Exam 11: Stellar Explosions
Exam 1: The Night Sky88 Questions
Exam 2: Light and Telescopes111 Questions
Exam 3: The Solar System109 Questions
Exam 4: Earth and Its Moon108 Questions
Exam 5: The Eight Planets112 Questions
Exam 6: Small Bodies in the Solar System108 Questions
Exam 7: Formation of Planetary Systems84 Questions
Exam 8: The Sun95 Questions
Exam 9: Measuring the Stars86 Questions
Exam 10: Star Formation and Evolution85 Questions
Exam 11: Stellar Explosions101 Questions
Exam 12: Black Holes77 Questions
Exam 13: The Milky Way Galaxy82 Questions
Exam 14: Galaxies98 Questions
Exam 15: Cosmology and the Universe98 Questions
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Novae always occur in a close binary star system.
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Looking at the elements that make up our world, which are the products of low versus high mass stars?
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Much of the lighter material in the Earth's crust and our bodies, such as carbon, oxygen, and nitrogen, is the product of low mass stars and given off in planetary nebula, type I supernovae, and stellar winds around giants. But the denser elements of the mantle and core, especially silicon and iron, are delivered to the interstellar medium from the cores of high mass stars by violent type II supernovae.
Iron is the most stably bonded atomic nucleus.
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The supernova that formed M-1, the Crab Nebula, was observed in
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An object more massive than the Sun, but roughly the size of a city, is a
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All neutron stars are pulsars, but not all pulsars are neutron stars.
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Compare the amount of time a 20 solar mass star will stay on the main sequence to the length of time its iron core can exist.
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Once carbon is formed in massive star cores, the majority of nuclei formed form then on will belong to even numbered elements, due to addition to more helium nuclei as alpha particles.
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Beyond the formation of iron, nuclear energy can be produced only by
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What would be most likely to disrupt the normal evolution of a star? Give examples of this.
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The maximum mass of a white dwarf is about ________ times the mass of the Sun.
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The density of a neutron star is comparable to the density of an atomic nucleus.
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The Crab Nebula and the Orion Nebula are regions where new stars are being formed.
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